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Title: Turbulence in core-collapse supernovae

Abstract

Multidimensional simulations show that non-radial, turbulent, fluid motion is a fundamental component of the core-collapse supernova explosion mechanism. Neutrino-driven convection, the standing accretion shock instability, and relic-perturbations from advanced nuclear burning stages can all impact the outcome of core collapse in a qualitative and quantitative way. Here, we review the current understanding of these phenomena and their role in the explosion of massive stars. We also discuss the role of protoneutron star convection and of magnetic fields in the context of the delayed neutrino mechanism.

Authors:
ORCiD logo [1];  [2];  [3];  [4];  [5];  [6]
  1. Inst. for Advanced Study, Princeton, NJ (United States). School of Natural Sciences; Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences
  2. Nazarbayev Univ., Astana (Kazakhstan). Dept. of Physics, School of Science and Technology
  3. California Inst. of Technology (CalTech), Pasadena, CA (United States). Walter Burke Inst. for Theoretical Physics
  4. Univ. of California, Berkeley, CA (United States). Dept. of Astronomy
  5. Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy, Dept. of Computational Mathematics, Science, and Engineering, and National Superconducting Cyclotron Lab.
  6. Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy, and National Superconducting Cyclotron Lab.
Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1523397
Grant/Contract Number:  
SC0015904; SC0017955; AC02-05CH11231; AC02-06CH11357
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Physics. G, Nuclear and Particle Physics
Additional Journal Information:
Journal Volume: 45; Journal Issue: 5; Journal ID: ISSN 0954-3899
Publisher:
IOP Publishing
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY

Citation Formats

Radice, David, Abdikamalov, Ernazar, Ott, Christian D., Mösta, Philipp, Couch, Sean M., and Roberts, Luke F. Turbulence in core-collapse supernovae. United States: N. p., 2018. Web. doi:10.1088/1361-6471/aab872.
Radice, David, Abdikamalov, Ernazar, Ott, Christian D., Mösta, Philipp, Couch, Sean M., & Roberts, Luke F. Turbulence in core-collapse supernovae. United States. doi:10.1088/1361-6471/aab872.
Radice, David, Abdikamalov, Ernazar, Ott, Christian D., Mösta, Philipp, Couch, Sean M., and Roberts, Luke F. Mon . "Turbulence in core-collapse supernovae". United States. doi:10.1088/1361-6471/aab872. https://www.osti.gov/servlets/purl/1523397.
@article{osti_1523397,
title = {Turbulence in core-collapse supernovae},
author = {Radice, David and Abdikamalov, Ernazar and Ott, Christian D. and Mösta, Philipp and Couch, Sean M. and Roberts, Luke F.},
abstractNote = {Multidimensional simulations show that non-radial, turbulent, fluid motion is a fundamental component of the core-collapse supernova explosion mechanism. Neutrino-driven convection, the standing accretion shock instability, and relic-perturbations from advanced nuclear burning stages can all impact the outcome of core collapse in a qualitative and quantitative way. Here, we review the current understanding of these phenomena and their role in the explosion of massive stars. We also discuss the role of protoneutron star convection and of magnetic fields in the context of the delayed neutrino mechanism.},
doi = {10.1088/1361-6471/aab872},
journal = {Journal of Physics. G, Nuclear and Particle Physics},
number = 5,
volume = 45,
place = {United States},
year = {2018},
month = {4}
}

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A new Multi-Dimensional General Relativistic Neutrino Hydrodynamics code for Core-Collapse Supernovae. iv. the Neutrino Signal
journal, May 2014


Gravitational wave Signatures of Magnetohydrodynamically Driven Core-Collapse Supernova Explosions
journal, November 2011


Supernova simulations from a 3D progenitor model – Impact of perturbations and evolution of explosion properties
journal, August 2017

  • Müller, Bernhard; Melson, Tobias; Heger, Alexander
  • Monthly Notices of the Royal Astronomical Society, Vol. 472, Issue 1
  • DOI: 10.1093/mnras/stx1962

General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae
journal, April 2013

  • Ott, Christian D.; Abdikamalov, Ernazar; Mösta, Philipp
  • The Astrophysical Journal, Vol. 768, Issue 2
  • DOI: 10.1088/0004-637X/768/2/115

Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
journal, September 2009


Chaos. ii. Gas-Phase Abundances in ngc 5194
journal, July 2015

  • Croxall, Kevin V.; Pogge, Richard W.; Berg, Danielle A.
  • The Astrophysical Journal, Vol. 808, Issue 1
  • DOI: 10.1088/0004-637X/808/1/42

Early Supernova Luminosity
journal, August 1969

  • Colgate, Stirling A.; McKee, Chester
  • The Astrophysical Journal, Vol. 157
  • DOI: 10.1086/150102

Implicit large eddy simulations of anisotropic weakly compressible turbulence with application to core-collapse supernovae
journal, August 2015

  • Radice, David; Couch, Sean M.; Ott, Christian D.
  • Computational Astrophysics and Cosmology, Vol. 2, Issue 1
  • DOI: 10.1186/s40668-015-0011-0

Electron-capture and Low-mass Iron-core-collapse Supernovae: New Neutrino-radiation-hydrodynamics Simulations
journal, November 2017

  • Radice, David; Burrows, Adam; Vartanyan, David
  • The Astrophysical Journal, Vol. 850, Issue 1
  • DOI: 10.3847/1538-4357/aa92c5

The Dominance of Neutrino-Driven Convection in Core-Collapse Supernovae
journal, June 2013

  • Murphy, Jeremiah W.; Dolence, Joshua C.; Burrows, Adam
  • The Astrophysical Journal, Vol. 771, Issue 1
  • DOI: 10.1088/0004-637X/771/1/52

The Nonmonotonic Dependence of Supernova and Compact Remnant Formation on Progenitor Rotation
journal, August 2005

  • Akiyama, Shizuka; Wheeler, J. Craig
  • The Astrophysical Journal, Vol. 629, Issue 1
  • DOI: 10.1086/431322

Is Strong sasi Activity the key to Successful Neutrino-Driven Supernova Explosions?
journal, August 2012


Bottleneck phenomenon in developed turbulence
journal, April 1994


Hydrodynamics of Core-Collapse Supernovae at the Transition to Explosion. i. Spherical Symmetry
journal, April 2012


The Spherical Accretion Shock Instability in the Linear Regime
journal, May 2006

  • Blondin, John M.; Mezzacappa, Anthony
  • The Astrophysical Journal, Vol. 642, Issue 1
  • DOI: 10.1086/500817